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Announcements of Upcoming Meetings

Notice that this list is not meant to be all-inclusive, but concentrates on meetings of potential interest to X-ray, gamma-ray, cosmic-ray, and gravitational astrophysicists. The HEASARC also maintains a list of on-line proceedings of high-energy astrophysics meetings. Updates, corrections, and/or suggestions about meetings should be sent to drake@olegacy.gsfc.nasa.gov

Other Sources of Information on Upcoming Meetings

Liz Bryson's list of International Astronomy meetings
Jet Propulsion Laboratory (JPL) Space Calendar


High Energy Astrophysics meetings

2009 September 7 - 11: X-ray Astronomy 2009: Present Status, Multiwavelength Approach and Future Perspectives

2009 September 11 - 12: Black Holes in Binary Systems: Observations versus Theory

2009 September 14 - 18: The Shocking Universe: Gamma-Ray Bursts and High-Energy Shock Phenomena in the Universe

2009 September 21: Chandra Calibration Review

2009 September 22 - 25: Ten Years of Science with Chandra: Chandra's First Decade of Discovery

2009 October 4 - 8: 4th INTERNATIONAL WORKSHOP ON ASTRONOMY AND RELATIVISTIC ASTROPHYSICS: New Phenomena and New States of Matter in the Universe in the AUGER, SLAC, LHC, FERMI, FAIR/GSI and GEO/LIGO Era

2009 October 7 - 9: Science with the New Generation of High Energy Gamma-ray Experiments: SCINEGHE-VII Workshop

2009 October 13 - 17: INTEGRAL Workshop: The Extreme Sky: Sampling the Universe above 10 keV

2009 November 2 - 5: 2009 Fermi Symposium

2009 November 17 -20: Swift Mission Conference: Celebrating 5 Years

2010 March 1 - 4: High Energy Astrophysics Division (HEAD) Meeting

2010 March 15 - 17: High-Resolution X-ray Spectroscopy: Past, Present, and Future

2010 May 24 - 26: Ultra-Luminous X-Ray Sources and Middle-Weight Black Holes

2010 July 18 - 25: 38th Scientific Assembly of the Committee on Space Research (COSPAR) and Associated Events: COSPAR 2010


Other Selected Astronomy, Physics and Space Science meetings

2009 October 26 - 28: Reionization to Exoplanets: Spitzer's Growing Legacy

2010 January 3 - 7: American Astronomical Society Meeting 215

2010 May 23 - 27: American Astronomical Society Meeting 216

2011 January 9 - 13: American Astronomical Society Meeting 217

2011 May 22 - 26: American Astronomical Society Meeting 218


Selected Astronomy-related Technology (e.g., Detectors) meetings


Selected Astronomy-related Physics, Computational, Data Analysis, Software or Statistics meetings


Selected Space Science-related Education and Public Outreach meetings


High Energy Astrophysics meetings

X-ray Astronomy 2009: Present Status, Multiwavelength Approach and Future Perspectives

Dates: 2009 September 7 - 11
(Extended) Deadline for Early Registration and Abstract Submission: 2009 May 15
Deadline for Final Registration: 2009 July 1
Place: Bologna, Italy

Third in a decadal series of X-ray astronomy conferences in Bologna, this meeting will highlight the contribution of XMM-Newton and Chandra observatories, ten years after their launch. Emphasis will be given on cosmic source multiwavelength studies and associated synergies with major facilities at all wavelengths, and on the perspectives for future high energy astrophysics missions.

The main scientific issues to be addressed are:

* STELLAR OBJECTS AND SUPERNOVA REMNANTS

	 - Cool and hot stars
	 - Star-forming regions 
	 - Neutron Stars
	 - Supernovae and SN remnants and pulsar wind nebulae
	 - Pulsars and Soft Gamma-Ray Repeaters 

* BLACK HOLES AND COMPACT OBJECTS  

        - Matter under extreme conditions 
        - Physics of Accretion and Ejection
	- X-rays as probes of General Relativity
	- Particle acceleration   
        - Evolution of Super-massive Black Holes
	- Black Hole-Galaxy Co-Evolution and Feedback processes

* GALAXIES AND CLUSTERS OF GALAXIES 

	-  Star formation across cosmic time 
	-  Physical processes in clusters and groups 
	-  Metal enrichement of the ICM 
	-  Interaction of cluster components 
	-  WHIM 
	-  Clusters of galaxies as cosmological probes

* PRESENT and FUTURE MISSIONS 

	- XMM, Chandra, Suzaku  
	- RossiXTE, INTEGRAL, Swift 
	- Simbol X, NuStar, EXIST, ASTRO-H
	- JANUS, GEMS, WFXT 
	- IXO 
	- Synergies with other wavelengths.

Black Holes in Binary Systems: Observations versus Theory

Dates: 2009 September 11 - 12
Deadline for Submission of Contributions: 2009 July 15
Place: Ferrara, Italy

The main goal of this workshop is to establish the current state of art in our understanding of the Physics of Black Hole sources, their spectral and timing signatures and to formulate the key fundamental problems of BH Physics and General Relativity, which can be addressed by future X-ray spectroscopic, timing and polarimetry missions.

Topics of the Workshop are:

  *  Spectra and variability of black-hole binaries
  *  Towards the measurement of fundamental parameters
  *  Spectral features, hard tails and annihilation lines
  *  Expectations from X-ray polarimetric observations of BH candidates. 

The Shocking Universe: Gamma-Ray Bursts and High-Energy Shock Phenomena in the Universe

Dates: 2009 September 14 - 18
Late Registration: Still Open
Place: San Servolo, Venice, Italy

The main themes of the meeting will be GRBs and high-energy relativistic shocks in the Universe. In addition to the large amount of unique data collected by Swift and by ground-based observatories, we have now the contribution of the Fermi satellite that, together with AGILE, will lead to many breakthroughs in these fields. GRB theories are likely to be at a turning point: the meeting itself will be a place where to witness the state of the art and evaluate new understanding and ideas. This would be extremely useful for all the community and in particular for the young participants and students.

The most recent literature tell us that we may have a problem with the standard internal shock scenario so that we will take a very critical view of the models with Meszaros, Piran and Kumar among others. Klebesadel will tell about the pioneering observations of the GRBs and later, getting into the core of the problems, we will develop new understanding following the latest observations and theoretical developments. Atwood, Meegan, Michelson and Ritz, among others, will cover some basic science relating it to the excellent data obtained with the Fermi satellite. A wide discussion about the physics of GRBs, their progenitors and environment will be led by Freyer, Ramirez-Ruiz, Berger and others. The meeting will also focus on the relation between SNe and GRBs.

A new, intriguing issue related to the study of GRBs is the possibility, in the near future, of detecting the emission of neutrinos and gravitational waves during the merging of NS - NS stars and the collapse of massive star. This requires accurate models necessary both for planning the observational strategies (and possibly new instruments) and for robust interpretation of future data. To this end, scientists from different research fields will present their work stimulating discussion and new ideas.

Chandra Calibration Review

Dates: 2009 September 21
Place: Boston, Massachusetts, USA

The Chandra Calibration Review (CCR) is held in order to disseminate and advance our understanding of the performance and capabilities of the Chandra X-ray Observatory. It is intended to share the Chandra teams' knowledge of the detectors, gratings, mirrors, and aspect system with the community while encouraging participation and feedback in the process of calibrating the observatory. Reports are solicited on various aspects of Chandra calibration.

This year, we will be holding the Calibration Review in conjunction with the Chandra's First Decade of Discovery symposium at the Seaport Hotel in Boston, Massachusetts. Calibration talks will be presented on Monday September 21, and calibration-related posters will be displayed throughout the symposium, which runs from Tuesday, September 22 through Friday, September 25.

Registration for the CCR is free and available through the Chandra's First Decade of Discovery website.

Ten Years of Science with Chandra: Chandra's First Decade of Discovery

Dates: 2009 September 22 - 25
Deadline for Oral Presentation Abstracts: 2009 July 10
Deadline for Other Abstracts and Hotel Reservations: 2009 August 21
Deadline for General and Student Registration: 2009 September 4
Place: Boston, Massachusetts, USA

This will be the fifth symposium in a series highlighting unique imaging and spectroscopic results from NASA's Chandra X-Ray Observatory. This event will celebrate key science results from the first ten years of operation of the Chandra X-ray Observatory. The focus will be on results which have had the largest impact on Astrophysics, including: The Cosmic Evolution of AGN, AGN outflows, evolutionary processes in clusters of galaxies, source populations and diffuse emission from normal galaxies, physical processes at the Galactic center, high spatial and spectral studies of neutron star physics, supernova remnants and star forming regions. It will also cover recent results from the XMM-Newton, Suzaku, Fermi Swift, INTEGRAL, RXTE and AGILE missions, as well as related theoretical results.

4th INTERNATIONAL WORKSHOP ON ASTRONOMY AND RELATIVISTIC ASTROPHYSICS (IWARA 2009): New Phenomena and New States of Matter in the Universe in the AUGER, SLAC, LHC, FERMI, FAIR/GSI and GEO/LIGO Era

Dates: 2009 October 4 - 8
Registrations and Contributions to this Event are now Closed
Place: Maresias, Sao Paulo, Brazil

The main purpose of the event is to offer new opportunities for personal and professional growth of our students. For this reason, we feel it is very important to keep the series of meetings that began in 2003 in which astrophysicists, astronomers and scientists working in nuclear, and high-energy particle physics, for the first time in this series, meet with the intention of showing the latest results on a variety of topics involving new phenomena and new states of matter in the universe and therefore interact with their peers from around the world. The previous IWARA meetings were in 2003 (Olinda, Pernambuco, Brazil), 2005 (Natal, Rio Grande do Norte, Brazil), and 2007, Joao Pessoa, Paraiba, Brazil).

"New Phenomena and New States of Matter in the Universe' is the motto of this event. The topics of the workshop include General Relativity, Gravitation, Cosmology, Heavy Ion Collisions and the Quark-Gluon Plasma, White Dwarfs, Neutron Stars and Pulsars, Black Holes, Gamma Ray Bursts, High-Energy Cosmic Rays, Gravitational Waves, Dark Matter and Dark Energy, Strange Matter and Strange Stars, Antimatter and Ion Research, and Cosmic Matter in the Laboratory. Related topics are welcome.

Science with the New Generation of High Energy Gamma-ray Experiments: SCINEGHE-VII Workshop

Dates: 2009 October 7 - 9
Deadline for Registration: mid-September
Place: Assisi, Perugia, Italy

This is the seventh workshop in a series after six successful editions in Perugia (2003), Bari (2004), Cividale del Friuli (2005), Elba Island (2006), Villa Mondragone (2007) and Padova (2008).

Fundamental research on the nature of matter at the high energy frontier takes place in three main fields: accelerator-based particle physics, high energy astrophysics, and the cosmology of the early universe. The study of astroparticle physics can have significant implications for collider physics at the LHC, and, at the same time, the LHC project provides the laboratory to perform measurements of great importance for cosmic ray astrophysics and cosmology. By the end of this year the Large Hadron Collider will begin taking data and start the exploration of the TeV scale physics and of the physics beyond the Standard Model. The Fermi Gamma-Ray Space Telescope mission has started in June 2008 and, after nearly one year of excellent performance on orbit, is producing a huge number of physics results, some of them already published and many more will be available by the time of the workshop. Interesting results will be also available from PAMELA, ATIC and Auger on cosmic ray physics. Ground based experiments (HESS, MAGIC, VERITAS, MILAGRO and ARGO) have been observing photons at the TeV scale with unprecedented accuracy and will also provide new results for the incoming years. Finally neutrino experiments and underground experiments for direct observation of dark matter and neutrino mass measurement are doing rapid progress.

The workshop will be distributed over 3 days, aiming to bring together researchers with different scientific backgrounds, High Energy Physics and High Energy Astrophysics, to share interests and to exchange new results in the various fields. Participation and abstract submission of young researchers and PhD students are strongly encouraged.

INTEGRAL Workshop: The Extreme Sky: Sampling the Universe above 10 keV

Dates: 2009 October 13 - 17
Start of Online Registration: 2009 June 15
Deadline for Abstract Submission of Contributed Talks/Posters: 2009 August 15
Place: Otranto (Lecce), Italy

All-sky surveys form the foundation of observational astronomy as they provide:

    * statistics on the types and distribution of celestial objects which 
         populate the Galaxy and the Universe
    * the ability to discover new classes of sources
    * a means of selecting specific types of objects for further 
         studies/observations

With respect to other surveys, those at high energies (above 10 keV) are particularly interesting as they probe the energy domain where fundamental changes from thermal to non-thermal sources/phenomena are expected, where the effects of absorption are drastically reduced, and a clearer picture of the Universe is possible. This is also the energy range where most of the extreme astrophysical behaviour is taking place, e.g. cosmic acceleration, explosions and accretion onto black holes and neutron stars. Recently a number of surveys have been performed in the keV to TeV energy range.

The objective of this workshop is to gather all the knowledge collected so far above 10 keV, to compare and contrast the results obtained in the various bands in the light of physical models and ultimately provide indications for future progress. The meeting is aimed at bringing together scientists active across the high energy range in order to focus on the opportunities offered by this new window both from the observational and theoretical viewpoints, while a dedicated section will also be devoted to discuss future mission ideas. The meeting will consist of invited talks and contributions which are welcome as either posters or as short interventions. There will be time for open discussions throughout. Finally, this meeting is a perfect way in which to celebrate with friends and colleagues INTEGRAL's 7th birthday and 7 years of success in gamma-ray astronomy.

The workshop will be organized in sessions dedicated to:

    * The soft gamma-ray sky: Surveys and observations from: INTEGRAL, SWIFT, 
          SUZAKU, MAXI etc
    * The high energy gamma-ray sky: Surveys and observations from: AGILE, 
          FERMI, HESS, MAGIC etc
    * The search for counterparts: Synergies between surveys: 
          The multi-waveband approach
    * Comparing and contrasting the two skies: Similarities and differences: 
          which theoretical implications, New source typologies: 
          what have we learnt
    * Prospects for future missions above 10 keV: Decadal Survey, Cosmic 
          Vision national programs etc.

2009 Fermi Symposium

Dates: 2009 November 2 - 5
Place: Washington, DC, USA

The 2009 Fermi Symposium is dedicated to results and prospects for scientific exploration of the Universe with the Fermi Gamma-ray Space Telescope and related studies. The symposium comes shortly after the Fermi data release, offering an opportunity for the astrophysical community to share in the excitement of discoveries being made with the Fermi instruments. Topics include: blazars and other active galactic nuclei, pulsars, gamma-ray bursts, supernova remnants, diffuse gamma radiation, unidentified gamma-ray sources, and searches for dark matter. The meeting will be held in downtown Washington, D.C,. near the U.S. Capitol Building.

Swift Mission Conference: Celebrating 5 Years

Dates: 2009 November 17 - 20
Deadline for Early Registration: 2009 October 1
Place: State College, Pennsylvania, USA

The goal of the Swift Mission Conference is to bring together scientists who have worked with Swift data in the last five years to talk about science results and discuss strategies for the future.

Swift is a highly successful NASA mission. Although Swift's primary task still is to observe gamma-ray bursts, it is one of the most versatile missions ever flown. With its multiwavelength and fast-scheduling capacity, the mission is ideal for multiwavelength and/or monitoring programs. Thus, it has been used for AGNs, supernovae, variable stars, transients, comets, and other phenomena. Swift has observed the closest objects (comets) and, with GRB 050904, 080913, and 090423, some of the most distant objects in the universe.

The future will bring new opportunities for Swift with increasing capacities in the GeV and TeV energy ranges from Fermi, AGILE, VERITAS, MAGIC, and HESS, and with gravitational wave detectors such as LIGO, VIRGO, and GEO, and the neutrino detectors ICECUBE and ANTARES.

High Energy Astrophysics Division (HEAD) of the AAS Meeting

Dates: 2010 March 1 - 4
Place: Hawaii, USA

High-Resolution X-ray Spectroscopy: Past, Present, and Future

Dates: 2010 March 15-17
Deadline for Abstract Submission: 2009 November 1
Deadline for Regular Registration: 2010 January 15
Deadline for Late Registration: 2010 March 1
Place: Utrecht, The Netherlands

High-resolution X-ray spectroscopy has become a powerful tool for astrophysics since the launch of Chandra and XMM-Newton, now 10 years ago. The grating spectrometers on both instruments still continue to provide excellent data, while imaging calorimeters are being prepared for future missions like Astro-H and IXO. The synergy with other wavelength bands like the UV will be boosted by the addition of COS to HST. X-ray spectroscopy offers unique diagnostics to study almost any object in the Universe. In this meeting we foresee presentations on highlights and the state-of-the-art of X-ray spectroscopy for a broad range of objects and on the prospects for future studies.

Ultra-Luminous X-Ray Sources and Middle-Weight Black Holes

Dates: 2010 May 24 - 26
Place: Villafranca, near Madrid, Spain

Tha aim of the workshop is to explore the physical nature of ultra-luminous X-ray sources (ULXs) and their connection to intermediate-mass black holes (IMBHs). Theorists and observers from the cosmology, X-ray, stellar dynamics, and AGN communities will be invited to explore topics of common interest, review new and recent results, and discuss the impact of upcoming observatories and space missions for black hole research.

38th Scientific Assembly of the Committee on Space Research (COSPAR) and Associated Events: COSPAR 2010

Dates: 2010 July 18 - 25
First Date for Abstract Submission: 2009 August 21
Deadline for Abstract Submission: 2010 February 19
Place: Bremen, Germany

Topics of COSPAR 2010 include:

Approximately 90 meetings covering the fields of COSPAR Scientific
Commissions (SC) and Panels:
- SC A:  The Earth's Surface, Meteorology and Climate 
- SC B:  The Earth-Moon System, Planets, and Small Bodies of the Solar System
- SC C:  The Upper Atmospheres of the Earth and Planets Including Reference 
         Atmospheres
- SC D:  Space Plasmas in the Solar System, Including Planetary Magnetospheres 
- SC E:  Research in Astrophysics from Space 
- SC F:  Life Sciences as Related to Space 
- SC G:  Materials Sciences in Space 
- SC H:  Fundamental Physics in Space 
- Panel on Satellite Dynamics (PSD)
- Panel on Scientific Ballooning (PSB)
- Panel on Potentially Environmentally Detrimental Activities in Space (PEDAS)
- Panel on Radiation Belt Environment Modelling (PRBEM)
- Panel on Space Weather (PSW)
- Panel on Planetary Protection (PPP)
- Panel on Capacity Building (PCB)
- Panel on Education (PE)
- Panel on Exploration (PEX)
- Special events:  Interdisciplinary lectures, space agency round table, etc.

For further details, contact:

The COSPAR Secretariat, 
c/o CNES, 2 place Maurice Quentin, 
75039 Paris Cedex 01, 
France 
Tel:     +33 1 44 76 75 10 
Fax:     +33 1 44 76 74 37
Email:   cospar@cosparhq.cnes.fr 
Website: http://www.cospar-assembly.org/

Other Selected Astronomy, Physics and Space Science meetings

Reionization to Exoplanets: Spitzer's Growing Legacy

Dates: 2009 October 26 - 28
Deadline for Early Registration: 2009 August 15
Deadline for Late Off-Site Registration: 2009 October 16
Place: Pasadena, California, USA

The 2009 Spitzer Science Center Conference, 'Reionization to Exoplanets: Spitzer's Growing Legacy', will occur shortly after the end of Spitzer's highly successful cryogenic mission, and at the start of the Spitzer warm mission. The meeting will celebrate the accomplishments of the cryogenic mission, and assess future opportunities in the fields where Spitzer's impact has been greatest. In particular, the meeting will be organized into five half day sessions, with each session focusing on a single science topic. The five session topics are:

1. Exoplanets and Exoplanetary Systems (planets, atmospheres, planetary systems, solar system)
2. Star Formation (molecular cloud cores, protoplanetary and debris disks, planet formation)
3. The Early Universe (structure and galaxy formation, young galaxies, star formation, stellar populations)
4. The Dusty Universe (nearby galaxies, starbursts, (U)LIRGs, sub-mm galaxies, AGNs)
5. The Galaxy (Galactic structure, interstellar medium).

In support of the Warm Spitzer mission, all Spitzer Cycle 6 Exploration Science teams are invited to hold team meetings during the conference. Please send the organizers an email to reserve space and time for your special break-out session. Meeting space for other Spitzer-related teams that wish to hold team meetings during the conference will be provided on an "as available" basis.

The oral program will consist entirely of invited reviews. All other attendees are urged to submit poster presentations on any aspect of astrophysical theory or observations related to the Spitzer mission.

American Astronomical Society Meeting 215

Dates: 2010 January 3 - 7
Place: Washington, DC, USA

American Astronomical Society Meeting 216

Dates: 2010 May 23 - 27
Place: Miami, Florida, USA

American Astronomical Society Meeting 217

Dates: 2011 January 9 - 13
Place: Seattle, Washington, USA

American Astronomical Society Meeting 218

Dates: 2011 May 22 - 26
Place: Boston, Massachusetts, USA

Selected Astronomy-related Technology (e.g., Detectors) meetings

None

Selected Astronomy-related Physics, Computational, Data Analysis, Software or Statistics meetings

None

Selected Space Science-related Education and Public Outreach meetings

None


Page Author: Stephen Drake


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Last modified: Tuesday, 11-Aug-2009 08:40:42 EDT